Results 51 to 60 of about 131,089 (321)

Population Properties of Neutron Stars in the Coalescing Compact Binaries

open access: yesThe Astrophysical Journal, 2021
Abstract We perform a hierarchical Bayesian inference to investigate the population properties of the coalescing compact binaries involving at least one neutron star (NS). With the current gravitational-wave (GW) observation data, we can rule out none of the double Gaussian, single Gaussian, and uniform NS mass distribution models ...
Yin-Jie 银杰 Li 李   +6 more
openaire   +2 more sources

Ultracompact X-ray binaries with He star companions [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT Ultracompact X-ray binaries (UCXBs) are low-mass X-ray binaries with hydrogen-deficient mass donors and ultrashort orbital periods. They have been suggested to be the potential Laser Interferometer Space Antenna (LISA) sources in the low-frequency region. Several channels for the formation of UCXBs have been proposed so far.
Bo Wang   +7 more
openaire   +2 more sources

CHIME Discovery of a Binary Pulsar with a Massive Nondegenerate Companion

open access: yesThe Astrophysical Journal, 2023
Of the more than 3000 radio pulsars currently known, only ∼300 are in binary systems, and only five of these consist of young pulsars with massive nondegenerate companions.
Bridget C. Andersen   +27 more
doaj   +1 more source

The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems [PDF]

open access: yes, 2015
We present several arguments which favor the scenario of two coexisting families of compact stars: hadronic stars and quark stars. Besides the well known hyperon puzzle of the physics of compact stars, a similar puzzle exists also when considering delta ...
Drago, Alessandro   +3 more
core   +2 more sources

Strange quark stars in binaries: formation rates, mergers and explosive phenomena [PDF]

open access: yes, 2017
The existence of strange quark stars has been proposed many years ago. More recently, the possible co-existence of a first family composed of "normal" neutron stars with a second family of strange quark stars has been proposed as a solution of problems ...
Drago, Alessandro   +3 more
core   +1 more source

A microquasar shot out from its birth place [PDF]

open access: yes, 2004
We show that the microquasar LSI+61303 is running away from its birth place in a young complex of massive stars. The supernova explosion that formed the compact object shot out the x-ray binary with a linear momentum of 430 +/- 140 Msun km/s, which is ...
Balberg   +35 more
core   +2 more sources

Dynamic normalization for compact binary coalescence searches in non-stationary noise [PDF]

open access: yesClassical and quantum gravity, 2020
The output of gravitational-wave interferometers, such as LIGO and Virgo, can be highly non-stationary. Broadband detector noise can affect the detector sensitivity on the order of tens of seconds. Gravitational-wave transient searches, such as those for
S. Mozzon   +15 more
semanticscholar   +1 more source

Great Impostors: Extremely Compact, Merging Binary Neutron Stars in the Mass Gap Posing as Binary Black Holes. [PDF]

open access: yesPhysical Review Letters, 2019
Can one distinguish a binary black hole undergoing a merger from a binary neutron star if the individual compact companions have masses that fall inside the so-called mass gap of 3-5  M_{⊙}?
A. Tsokaros   +4 more
semanticscholar   +1 more source

startrack predictions of the stochastic gravitational-wave background from compact binary mergers [PDF]

open access: yesPhysical Review D, 2020
We model the gravitational-wave background created by double compact objects from isolated binary evolution across cosmic time using the startrack binary population code.
C. Périgois   +3 more
semanticscholar   +1 more source

Population Synthesis of Black Hole Binaries with Compact Star Companions [PDF]

open access: yesThe Astrophysical Journal, 2021
Abstract We perform a systematic study of merging black hole (BH) binaries with compact star (CS) companions, including black hole–white dwarf (BH–WD), black hole–neutron star (BH–NS), and black hole–black hole (BH–BH) systems. Previous studies have shown that mass transfer stability and common envelope evolution can significantly affect
Yong Shao, Xiang-Dong Li
openaire   +2 more sources

Home - About - Disclaimer - Privacy